Near Infrared Spectroscopy as a Probe of Excitation in Star Formation Regions

Details Near Infrared Spectroscopy as a Probe of Excitation in Star Formation Regions Near Infrared Spectroscopy as a Probe of Excitation in Star Formation Regions

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..103l&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

Astronomy and Astrophysics

Astronomy

Scientific paper

The only bright recombination lines from HII regions in the
near-infrared JHK wavebands are due to hydrogen and helium. This paper
outlines the potential uses and problems with these lines in setting
limits on the form of the emergent ultraviolet stellar radiation field.

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